The neutrino-nucleon cross section at UHE and its astrophysical implications
arXiv:1505.06583 · doi:10.1103/PhysRevD.92.014027
Abstract
We present a quantitative study of the cross section in the neutrino energy range GeV within two transversal QCD approaches: NLO DGLAP evolution using different sets of PDFs and BK small- evolution with running coupling and kinematical corrections. We show that the non-linear effects embodied in the BK equation yield a slower raise in the cross section for GeV than the usual DGLAP based calculation. Finally, we translate this theoretical uncertainty into upper bounds for the ultra-high-energy neutrino flux for different experiments.
17 pages; 5 figures. References and comments added
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